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Neurologische Pharmakotherapie: Buchbesprechung
In: Neurotransmitter, Volume 25, Issue S13, p. 26-26
ISSN: 2196-6397
Individuelle reflexive Werte
Der Fragebogen erfasst die individuellen reflexiven Werte einer Person. Dabei unterteilt Hermann das Konstrukt in neun Faktoren: "Subkulturell-materialistische Orientierung", "Hedonistische Orientierung", "Sozialintegrative Orientierung", "Sozialer Altruismus", "Ökologisch-alternative Orientierung", "Politisch tolerante Orientierung", "Normorientierte Leistungsethik", "Konservativer Konformismus", "Religiöse Orientierung".
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Supervised Disulfiram in Relapse Prevention in Alcohol-Dependent Patients Suffering From Comorbid Borderline Personality Disorder--A Case Series
In: Alcohol and alcoholism: the international journal of the Medical Council on Alcoholism (MCA) and the journal of the European Society for Biomedical Research on Alcoholism (ESBRA), Volume 45, Issue 2, p. 146-150
ISSN: 1464-3502
Das handlungsbuch von Hermann und Johann Wittenborg
In: http://hdl.handle.net/2027/wu.89097368104
Familie und politische persönlichkeit Johann Wittenborgs.--Das handlungsbuch.--Die buchführung.--Gesellschaften und sendeve.--Das geschäft Johann Wittenborgs.--Makler, handelsmarken, spesen.--Münzen.--Das handlungsbuch Hermann Wittenborgs.--Das handlungsbuch Johann Wittenborgs.--Briefe.--Auszüge aus dem Oberstadtbuch.--Auszüge aus dem Niederstadtbuch.--Testamente und urkunden. ; Mode of access: Internet.
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REWARD CRAVING AND WITHDRAWAL RELIEF CRAVING: ASSESSMENT OF DIFFERENT MOTIVATIONAL PATHWAYS TO ALCOHOL INTAKE
In: Alcohol and alcoholism: the international journal of the Medical Council on Alcoholism (MCA) and the journal of the European Society for Biomedical Research on Alcoholism (ESBRA), Volume 38, Issue 1, p. 35-39
ISSN: 1464-3502
SY27-2RELAPSE VULNERABILITY AS A BRAIN NETWORK STATE: STUDIES IN HUMANS AND RATS
In: Alcohol and alcoholism: the international journal of the Medical Council on Alcoholism (MCA) and the journal of the European Society for Biomedical Research on Alcoholism (ESBRA), Volume 50, Issue suppl 1, p. i30.2-i30
ISSN: 1464-3502
OR2-1Low μu-Opioid Receptor Status in Alcohol Dependence Identified by Combined Positron Emission Tomography and Post-Mortem Brain Analysis
In: Alcohol and alcoholism: the international journal of the Medical Council on Alcoholism (MCA) and the journal of the European Society for Biomedical Research on Alcoholism (ESBRA), Volume 52, Issue suppl_1, p. i31-i49
ISSN: 1464-3502
CARMENES: high-resolution spectra and precise radial velocities in the red and infrared
The design and construction of CARMENES has been presented at previous SPIE conferences. It is a next-generation radial-velocity instrument at the 3.5m telescope of the Calar Alto Observatory, which was built by a consortium of eleven Spanish and German institutions. CARMENES consists of two separate échelle spectrographs covering the wavelength range from 0.52 to 1.71¿m at a spec-tral resolution of R < 80,000, fed by fibers from the Cassegrain focus of the telescope. CARMENES saw ¿First Light¿ on Nov 9, 2015. During the commissioning and initial operation phases, we established basic performance data such as throughput and spectral resolution. We found that our hollow-cathode lamps are suitable for precise wavelength calibration, but their spectra contain a number of lines of neon or argon that are so bright that the lamps cannot be used in simultaneous exposures with stars. We have therefore adopted a calibration procedure that uses simultaneous star / Fabry Pérot etalon exposures in combination with a cross-calibration between the etalons and hollow-cathode lamps during daytime. With this strategy it has been possible to achieve 1-2 m/s precision in the visible and 5-10 m/s precision in the near-IR; further improvements are expected from ongoing work on temperature control, calibration procedures and data reduction. Comparing the RV precision achieved in different wavelength bands, we find a ¿sweet spot¿ between 0.7 and 0.8¿m, where deep TiO bands provide rich RV information in mid-M dwarfs. This is in contrast to our pre-survey models, which predicted comparatively better performance in the near-IR around 1¿m, and explains in part why our near-IR RVs do not reach the same precision level as those taken with the visible spectrograph. We are now conducting a large survey of 340 nearby M dwarfs (with an average distance of only 12pc), with the goal of finding terrestrial planets in their habitable zones. We have detected the signatures of several previously known or suspected planets and also discovered several new planets. We find that the radial velocity periodograms of many M dwarfs show several significant peaks. The development of robust methods to distinguish planet signatures from activity-induced radial velocity jitter is therefore among our priorities. Due to its large wavelength coverage, the CARMENES survey is generating a unique data set for studies of M star atmospheres, rotation, and activity. The spectra cover important diagnostic lines for activity (H alpha, Na I D1 and D2, and the Ca II infrared triplet), as well as FeH lines, from which the magnetic field can be inferred. Correlating the time series of these features with each other, and with wavelength-dependent radial velocities, provides excellent handles for the discrimination between planetary companions and stellar radial velocity jitter. These data are also generating new insight into the physical properties of M dwarf atmospheres, and the impact of activity and flares on the habitability of M star planets. © 2018 SPIE. ; CARMENES is an instrument for the Centro Astronomico Hispano-Aleman de Calar Alto (CAHA, Almeria, Spain). CARMENES is funded by the German Max-Planck-Gesellschaft (MPG), the Spanish Consejo Superior de Investigaciones Cientificas (CSIC), the European Union through FEDER/ERF FICTS-2011-02 funds, and the members of the CARMENES Consortium (Max-Planck-Institut fur Astronomie, Instituto de Astrofisica de Andalucia, Landessternwarte Konigstuhl, Institut de Ciencies de l'Espai, Insitut fur Astrophysik Gottingen, Universidad Complutense de Madrid, Thuringer Landessternwarte Tautenburg, Instituto de Astrofisica de Canarias, Hamburger Sternwarte, Centro de Astrobiologia and Centro Astronomico Hispano-Aleman), with additional contributions by the Spanish Ministry of Science, the German Science Foundation through the Major Research Instrumentation Program and DFG Research Unit FOR2544 "Blue Planets around Red Stars", the Klaus Tschira Stiftung, the states of Baden-Wurttemberg and Niedersachsen, and by the Junta de Andalucia.
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